Cosmic Microwave Background Anisotropies: Inflation versus Topological Defects

Mairi Sakellariadou

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arXiv · astro-ph/9911497

Cosmic Microwave Background Anisotropies: Inflation versus Topological Defects

Mairi Sakellariadou

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Abstract

I present a briefly summary of the current status of inflationary models versus topological defects scenarios, as the mechanisms which could have induced the initial density perturbations, which left an imprint on the cosmic microwave backgound radiation anisotropies.

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Mairi Sakellariadou. 1999-11-29. Cosmic Microwave Background Anisotropies: Inflation versus Topological Defects. https://arxiv.org/abs/astro-ph/9911497

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